Discussion Overview
The discussion centers around identifying a comprehensive review paper on the observational status of astrophysical black holes, specifically seeking resources that cover both supermassive and solar-mass black holes. Participants express interest in recent developments and upcoming observational techniques, particularly related to Sgr A*.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- One participant requests a review paper that is up to date, freely available, and covers both supermassive and solar-mass black holes.
- Another participant suggests a paper focused solely on Sgr A*, noting its relevance to the discussion.
- A participant expresses surprise at the advancements in observations of Sgr A*, particularly regarding measurements probing its spin.
- There is a question about whether an all-encompassing review paper exists for both types of black holes, with speculation on the focus shifting to Sgr A* due to its accessibility for strong-field general relativity studies.
- A participant shares insights from a talk by Broderick, highlighting the expectation of VLBI images of Sgr A* resolving the event horizon within five years and comparing it to the black hole in Centaurus-A.
- Another participant calculates the distance required for a stellar mass black hole to subtend an angular size comparable to Sgr A*, suggesting challenges in imaging such black holes in the near future.
- A further suggestion for a paper is provided, although its relevance is not elaborated upon.
Areas of Agreement / Disagreement
Participants do not reach a consensus on a specific review paper that meets all criteria. There are multiple competing views regarding the focus on Sgr A* versus other black holes, and the discussion remains unresolved regarding the availability of a comprehensive review.
Contextual Notes
Participants express uncertainty about the availability of a review covering both supermassive and solar-mass black holes, and there are assumptions about the observational capabilities and distances involved in imaging stellar mass black holes.